| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.97 | 31.69 | 2.89 | 18.45 | -15.46 | 5.39 | 24.12 | 228.48 | 0.5278 | 338.9 | 346.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.87 | 0.00 | 0.51 | -15.04 | 7.50 | 26.22 | 231.47 | 0.5475 | 544.0 | 480.8 | |
| 0.00 | 1.48 | 0.00 | 0.88 | -15.63 | 7.06 | 25.78 | 230.15 | 0.5477 | 647.0 | 571.9 | |
| 2.79 | 8.62 | 1.63 | 5.05 | -15.03 | 6.47 | 25.19 | 230.38 | 0.5357 | 803.1 | 715.0 | |
| 0.00 | 1.31 | 0.00 | 0.76 | -14.71 | 6.39 | 25.11 | 230.78 | 0.5320 | 711.0 | 448.8 | |
| 0.00 | 1.48 | 0.00 | 0.87 | -15.56 | 6.19 | 24.91 | 229.30 | 0.5374 | 688.0 | 475.5 | |
| 0.00 | 0.35 | 0.00 | 0.20 | -15.68 | 6.07 | 24.79 | 228.98 | 0.5372 | 605.0 | 609.8 | |
| 0.00 | 1.74 | 0.00 | 1.02 | -15.84 | 5.95 | 24.68 | 228.62 | 0.5374 | 864.0 | 683.3 | |
| 0.00 | 2.00 | 0.00 | 1.18 | -16.09 | 5.95 | 24.68 | 228.25 | 0.5398 | 622.0 | 512.0 | |
| 0.00 | 3.31 | 0.00 | 1.94 | -16.28 | 5.74 | 24.46 | 227.75 | 0.5391 | 826.0 | 563.1 | |
| 2.18 | 3.48 | 1.26 | 2.01 | -15.24 | 4.69 | 23.41 | 228.02 | 0.5178 | 832.0 | 673.7 | |
| 0.00 | 1.48 | 0.00 | 0.86 | -16.66 | 4.22 | 22.95 | 225.40 | 0.5267 | -698.0 | -424.1 | |
| 0.00 | 1.74 | 0.00 | 1.01 | -16.65 | 3.92 | 22.64 | 225.03 | 0.5233 | -278.0 | -290.2 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -13.91 | 2.88 | 21.60 | 227.79 | 0.4843 | -767.0 | -586.1 | |
| 0.00 | 1.22 | 0.00 | 0.69 | -15.05 | 2.16 | 20.89 | 225.08 | 0.4882 | -551.0 | -462.9 | |
| 0.00 | 1.65 | 0.00 | 0.93 | -14.61 | 1.16 | 19.89 | 224.37 | 0.4727 | -185.0 | -302.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |